New limits on light dark matter - proton cross section from the cosmic large-scale structure

Abstract

We set the strongest limits to-date on the velocity-independent dark matter (DM) - proton cross section $\sigma$ for DM masses $m=10\mathrm{keV}$ to $100\mathrm{GeV}$, using large-scale structure traced by the Lyman-alpha forest: e.g., a 95% lower limit $\sigma <6\times 10^{-30}{\mathrm{cm}}^2$, for $m=100\mathrm{keV}$. Our results complement direct detection, which has limited sensitivity to sub-GeV DM. We use an emulator of cosmological simulations, combined with data from the smallest cosmological scales used to-date, to model and search for the imprint of primordial DM-proton collisions. Cosmological bounds are improved by up to a factor of 25.

12 pages, 5 figures. Minor changes to match version accepted for publication in PRL

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